SDO HMI 2011-11-13 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.17 | 238.33 | 68.86 | 304.86 | -17.90 | 104.36 | 64.72 | 249.03 | 0.9212 | 89.9 | 39.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.44 | 90.72 | 12.14 | 131.74 | -17.18 | 107.48 | 67.84 | 250.44 | 0.9405 | 536.0 | 30.9 | |
| 1.46 | -1.00 | 2.09 | -1.00 | -17.76 | 107.18 | 67.55 | 249.78 | 0.9395 | 269.3 | 999999 | |
| 1.89 | -1.00 | 2.71 | -1.00 | -18.17 | 107.09 | 67.46 | 249.34 | 0.9394 | 299.2 | 999999 | |
| 2.32 | 17.30 | 3.23 | 23.57 | -17.79 | 106.55 | 66.92 | 249.63 | 0.9359 | 232.8 | 473.1 | |
| 0.77 | -1.00 | 1.10 | -1.00 | -18.45 | 106.99 | 67.35 | 249.02 | 0.9391 | 418.3 | 999999 | |
| 1.38 | -1.00 | 1.96 | -1.00 | -18.66 | 106.92 | 67.28 | 248.78 | 0.9390 | 482.9 | 999999 | |
| 2.58 | 11.62 | 3.75 | 16.80 | -19.19 | 107.27 | 67.64 | 248.30 | 0.9415 | 365.5 | 289.5 | |
| 1.46 | -4.00 | 1.98 | -4.00 | -17.95 | 105.96 | 66.32 | 249.35 | 0.9327 | 439.2 | 999999 | |
| 1.29 | -4.00 | 1.74 | -4.00 | -17.76 | 105.81 | 66.18 | 249.53 | 0.9316 | 625.1 | 999999 | |
| 0.00 | 1.55 | 0.00 | 2.12 | -18.46 | 106.03 | 66.40 | 248.83 | 0.9337 | 612.0 | 520.7 | |
| 2.41 | 4.05 | 3.19 | 5.34 | -17.92 | 105.31 | 65.68 | 249.26 | 0.9288 | 426.4 | 430.1 | |
| 2.50 | 4.48 | 3.31 | 5.94 | -18.33 | 105.31 | 65.67 | 248.82 | 0.9292 | 346.8 | 190.7 | |
| 1.21 | 2.24 | 1.55 | 2.89 | -18.20 | 104.61 | 64.97 | 248.82 | 0.9248 | 547.6 | 476.3 | |
| 0.00 | 1.38 | 0.00 | 1.66 | -16.50 | 103.27 | 63.64 | 250.37 | 0.9139 | -386.0 | -283.1 | |
| 0.00 | 3.10 | 0.00 | 3.91 | -18.33 | 104.03 | 64.40 | 248.56 | 0.9214 | 659.0 | 581.4 | |
| 0.52 | 1.46 | 0.68 | 1.91 | -19.94 | 104.56 | 64.93 | 246.96 | 0.9269 | -114.0 | -37.8 | |
| 0.00 | 0.60 | 0.00 | 0.78 | -19.77 | 104.20 | 64.57 | 247.07 | 0.9244 | -263.0 | -251.7 | |
| 4.56 | 19.19 | 5.41 | 22.59 | -17.65 | 102.45 | 62.82 | 248.95 | 0.9101 | 549.8 | 491.6 | |
| 0.00 | 1.55 | 0.00 | 2.02 | -20.42 | 104.41 | 64.78 | 246.43 | 0.9266 | -111.0 | -34.7 | |
| 1.81 | 3.18 | 2.32 | 4.08 | -20.30 | 104.10 | 64.46 | 246.48 | 0.9246 | -351.0 | -215.2 | |
| 0.00 | 1.89 | 0.00 | 2.33 | -19.96 | 102.97 | 63.33 | 246.59 | 0.9170 | -331.0 | -190.6 | |
| 0.00 | 0.52 | 0.00 | 0.59 | -17.68 | 101.26 | 61.62 | 248.65 | 0.9019 | 424.0 | 416.5 | |
| 0.00 | 1.21 | 0.00 | 1.39 | -18.52 | 101.57 | 61.94 | 247.81 | 0.9055 | -169.0 | -144.2 | |
| 0.00 | 1.46 | 0.00 | 1.70 | -19.19 | 101.60 | 61.97 | 247.10 | 0.9068 | -178.0 | -105.9 | |
| 0.00 | 1.21 | 0.00 | 1.43 | -19.85 | 101.98 | 62.34 | 246.48 | 0.9104 | 431.0 | 356.1 | |
| 1.03 | 3.18 | 1.16 | 3.57 | -19.07 | 100.53 | 60.90 | 246.97 | 0.8992 | -257.0 | -17.7 | |
| 1.21 | 1.89 | 1.27 | 2.00 | -17.30 | 99.12 | 59.49 | 248.56 | 0.8857 | -208.8 | -130.5 | |
| 0.00 | 0.95 | 0.00 | 1.02 | -18.26 | 99.53 | 59.90 | 247.60 | 0.8905 | 130.0 | 154.1 | |
| 1.29 | 2.15 | 1.37 | 2.29 | -18.27 | 99.04 | 59.40 | 247.47 | 0.8869 | -245.2 | -339.2 | |
| 5.59 | 7.57 | 6.13 | 8.30 | -19.54 | 99.67 | 60.03 | 246.24 | 0.8939 | -508.2 | -214.9 | |
| 3.96 | 47.17 | 4.06 | 47.76 | -17.18 | 98.09 | 58.46 | 248.43 | 0.8775 | -477.6 | -401.7 | |
| 2.50 | 5.59 | 2.68 | 6.00 | -19.13 | 99.10 | 59.47 | 246.54 | 0.8890 | -473.0 | -516.0 | |
| 4.99 | -31.00 | 5.03 | -31.00 | -17.16 | 97.54 | 57.91 | 248.31 | 0.8732 | -930.0 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.13 | -17.97 | 97.49 | 57.85 | 247.39 | 0.8744 | -453.0 | -395.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |